dataset for "Type Ia Supernovae Can Arise from the Detonations of Both Stars in a Double Degenerate Binary"

Included here are datafiles supplementary to the article "Type Ia Supernovae Can Arise from the Detonations of Both Stars in a Double Degenerate Binary", submitted to ApJ/arxiv in January 2024. For each model, there are files for their final nuclear yields, complete (non-decayed) ejecta in 2D velocity space (Sedona input format), and 2D spectra that are calculated out to around 50 days. Models are labeled based on their progenitor mass, i.e. the model involving the 1.00 solar mass primary and 0.90 solar mass companion is called "m100_m090". The model with the suffix 'nosecdet' has a companion, but it is not ignited.